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Uncommon neo 29 EP

5381 Sekhmet (1991 JY)

Position computed live · sbdb

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Live ephemeris

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Score breakdown

· 4 badges
29 pts · Uncommon
Uncommon 33 pts → Rare
  • Crosses Earth's orbit +12
  • Has a proper name +8
  • Near-Earth object +5
  • Tiny fragment (<1 km) +4
Total score 29

4 more points to reach Rare.

Badges

  • Near-Earth object · +5
  • Tiny fragment (<1 km) · +4
  • Crosses Earth's orbit · +12
  • Has a proper name · +8

Trivia

How we found it

  • Named. Notable enough to have earned a proper name, not just a catalogue number.

Cosmic context

  • Size. Roughly 0.9 km across.
  • Ancient. A leftover from the Solar System's birth, older than every continent on Earth.

Properties

diameter km
0.935
eccentricity
0.2964
h mag
16.75
inclination
48.97
name
5381 Sekhmet (1991 JY)
named
yes
orbit class
ATE
perihelion au
0.6667
semi major au
0.9475

About 5381 Sekhmet (1991 JY)

5381 Sekhmet (1991 JY) is an uncommon neo. It swings within 0.667 AU of the Sun at perihelion.

Roughly 0.9 km across.

How to see it

Like any astronomical target, 5381 Sekhmet (1991 JY) is best seen from a dark site away from city lights, and when it is above the horizon depends on your latitude and the time of year. Because it moves against the background stars, the live position panel on this page tracks where it is right now. The visibility panel above works out tonight's viewing window for your saved location.

Why 5381 Sekhmet (1991 JY) is an uncommon neo

5381 Sekhmet (1991 JY) scores 29 points on Spacedle's rarity scale, which places it in the uncommon tier. Another 4 points would lift it into a rarer tier.

That score comes from 4 science badges — Near-Earth object, Tiny fragment (<1 km), Crosses Earth's orbit and Has a proper name — each earned for a real, measurable property of the object. Rarity on Spacedle is never random: the more remarkable an object's astrophysics, the more badges it collects, the higher it scores, and the rarer it ranks.

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Sky imagery and survey data courtesy of Aladin Lite & CDS, Strasbourg. Object data from the NASA Exoplanet Archive, JPL Small-Body Database, and the ATNF Pulsar Catalogue.